Unveiling stellar magnetic activity using CoRoT seismic observations
It is well known that in the Sun, the frequencies and amplitudes of acoustic modes vary throughout the solar cycle. Indeed, while the magnetic activity goes...
Unveiling the sources of disk heating in spiral galaxies with the CALIFA survey
The stellar velocity ellipsoid (SVE) quantifies the amount of velocity dispersion in the vertical, radial and azimuthal directions. Since different disk heating...
Unveiling the Structure of the Planetary Nebula M2-48
The PN M2-48 is formed by three main structures, namely, a bipolar central region (CR), a set of knots tracing a semicircular shell surrounding CR, and two...
Update and preliminary performance analysis of the New Robotic Telescope structure
The New Robotic Telescope will be 4-meter class telescope with a fast response time (less than 30 seconds) as its primary design target. To achieve this, enough...
The STARE telescope of the High Altitude Observatory (HAO), Boulder is maintained by the Instituto de Astrofísica de Canarias (IAC) at the Observatorio del...
Update of FastCam, the lucky imaging instrument at the Observatorios de Canarias (OCAN)
FastCam is an instrument designed to obtain high spatial resolution images in the optical wave- length range from ground-based telescopes by using the Lucky...
The GTC project office is continuing to develop the plans for the commissioning of the GTC. The commissioning will start before first light, and will continue...